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Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/7829
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dc.contributor.authorKarmakar, Siddharthaen_US
dc.contributor.authorPandey, Sujataen_US
dc.contributor.authorRakshit, Subhenduen_US
dc.date.accessioned2022-03-17T01:00:00Z-
dc.date.accessioned2022-03-21T11:14:06Z-
dc.date.available2022-03-17T01:00:00Z-
dc.date.available2022-03-21T11:14:06Z-
dc.date.issued2021-
dc.identifier.citationKarmakar, S., Pandey, S., & Rakshit, S. (2021). Astronomy with energy dependent flavour ratios of extragalactic neutrinos. Journal of High Energy Physics, 2021(10) doi:10.1007/JHEP10(2021)004en_US
dc.identifier.issn1029-8479-
dc.identifier.otherEID(2-s2.0-85116397766)-
dc.identifier.urihttps://doi.org/10.1007/JHEP10(2021)004-
dc.identifier.urihttps://dspace.iiti.ac.in/handle/123456789/7829-
dc.description.abstractHigh energy astrophysical neutrinos interacting with ultralight dark matter (DM) can undergo flavour oscillations that induce an energy dependence in the flavour ratios. Such a dependence on the neutrino energy will reflect in the track to shower ratio in neutrino telescopes like IceCube or KM3NeT. This opens up a possibility to study DM density profiles of astrophysical objects like AGN, GRB etc., which are the suspected sources of such neutrinos. © 2021, The Author(s).en_US
dc.language.isoenen_US
dc.publisherSpringer Science and Business Media Deutschland GmbHen_US
dc.sourceJournal of High Energy Physicsen_US
dc.titleAstronomy with energy dependent flavour ratios of extragalactic neutrinosen_US
dc.typeJournal Articleen_US
dc.rights.licenseAll Open Access, Gold, Green-
Appears in Collections:Department of Physics

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